Search results for "Scintillation"

showing 10 items of 145 documents

Sub-nanosecond excitonic luminescence in ZnO:In nanocrystals

2019

The financial support of research European Union ERA.NET RUS_ST20170-51 . This work was partly supported by Russian Foundation for Basic Research, Russia , project No. 18-52-76002 . The sample preparation was carried out as part of SFERA II project -Transnational Access activities ( European Union 7th Framework Programme Grant Agreement N3126430 ).

010302 applied physicsRadiationMaterials scienceMorphology (linguistics)DopingKineticsAnalytical chemistrychemistry.chemical_elementTime-resolved luminescenceNanosecondVapour deposition01 natural sciences030218 nuclear medicine & medical imaging03 medical and health sciences0302 clinical medicineNanocrystalchemistry0103 physical sciences:NATURAL SCIENCES:Physics [Research Subject Categories]In [ZnO]Indium dopingLuminescenceInstrumentationScintillationIndium
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Measurements of underlying-event properties using neutral and charged particles in pp collisions at root s=900 GeV and root s=7 TeV with the ATLAS de…

2011

We present first measurements of charged and neutral particle-flow correlations in pp collisions using the ATLAS calorimeters. Data were collected in 2009 and 2010 at centre-of-mass energies of 900 GeV and 7 TeV. Events were selected using a minimum-bias trigger which required a charged particle in scintillation counters on either side of the interaction point. Particle flows, sensitive to the underlying event, are measured using clusters of energy in the ATLAS calorimeters, taking advantage of their fine granularity. No Monte Carlo generator used in this analysis can accurately describe the measurements. The results are independent of those based on charged particles measured by the ATLAS …

:Mathematics and natural science: 400::Physics: 430 [VDP]Physics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsMonte Carlo method:Mathematics and natural science: 400::Physics: 430::Nuclear and elementary particle physics: 431 [VDP]7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)JetsNaturvetenskap[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]QCATLAS detector; LHCPhysicsLarge Hadron ColliderSettore FIS/01 - Fisica SperimentaleATLASCharged particleCalorimetermedicine.anatomical_structureScintillation counterComputingMethodologies_DOCUMENTANDTEXTPROCESSINGDistributionsFísica nuclearLHCNatural Sciencespp collisionsParticle Physics - ExperimentParticle physicsCiências Naturais::Ciências Físicas:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesddc:500.2530Nuclear physicsAtlas (anatomy)0103 physical sciencesmedicineddc:530High Energy Physics010306 general physicsEngineering (miscellaneous)Ciencias ExactasCalorimeterHeraScience & Technologyneutral particle-flow correlationsInteraction point010308 nuclear & particles physicsFísicaQC0793Experimental High Energy PhysicsParticle
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Digital liquid-scintillation counting and effective pulse-shape discrimination with artificial neural networks

2014

Abstract A typical problem in low-level liquid scintillation (LS) counting is the identification of α particles in the presence of a high background of β and γ particles. Especially the occurrence of β-β and β-γ pile-ups may prevent the unambiguous identification of an α signal by commonly used analog electronics. In this case, pulse-shape discrimination (PSD) and pile-up rejection (PUR) units show an insufficient performance. This problem was also observed in own earlier experiments on the chemical behaviour of transactinide elements using the liquid-liquid extraction system SISAK in combination with LS counting. α-particle signals from the decay of the transactinides could not be unambigu…

Artificial neural networkAnalogue electronicsChemistrybusiness.industryLiquid scintillation countingPattern recognitionSignalPulse (physics)Artificial intelligenceTransient (oscillation)Physical and Theoretical ChemistryOscilloscopebusinessDigital recordingRadiochimica Acta
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Perspectives for CNO neutrino detection in Borexino

2018

International audience; Borexino measured with unprecedented accuracy the fluxes of solar neutrinos emitted at all the steps of the pp fusion chain. Still missing is the measurement of the flux of neutrinos produced in the CNO cycle. A positive measurement of the CNO neutrino flux is of fundamental importance for understanding the evolution of stars and addressing the unresolved controversy on the solar abundances. The measurement of the CNO neutrino flux in Borexino is challenging because of the low intensity of this component (CNO cycle accounts for about 1% of the energy emitted by Sun), the lack of prominent spectral features and the presence of background sources. The main background c…

CNO cycleexperimental methodsneutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical Phenomenascintillation counter: liquidSolar neutrinosbismuth: admixtureAstrophysics[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]7. Clean energySolar neutrinoCNO-cycleneutrino: fluxAstrophysics::Solar and Stellar Astrophysics[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Stellar evolutionBorexinoliquid scintillatorAstrophysics::Galaxy AstrophysicsPhysicsEnergy distributiondetectorbackgroundbismuth: nuclideCNO cycleNeutrino detector13. Climate actionBorexinoExperimental methodsNeutrino
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Searching for New Physics in two-neutrino double beta decay with CUPID

2021

Abstract In the past few years, attention has been drawn to the fact that a precision analysis of two-neutrino double beta decay (2υββ) allows the study of interesting physics cases like the emission of Majoron bosons and possible Lorentz symmetry violation. These processes modify the summed-energy distribution of the two electrons emitted in 2υββ. CUPID is a next-generation experiment aiming to exploit 100Mo-enriched scintillating Li2MoO4 crystals, operating as cryogenic calorimeters. Given the relatively fast half-life of 100Mo 2υββ and the large exposure that can be reached by CUPID, we expect to measure with very high precision the 100Mo 2υββ spectrum shape, reaching great sensitivities…

CUPID Neutrinoless Double Beta Decay LNGS Particle Physics Neutrino Majorana NeutrinoHistoryLNGS[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]hiukkasfysiikkaNeutrinoless Double Beta DecayEducationcrystalCUPIDNeutrino[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]double-beta decay: (2neutrino)Particle Physicsscintillation countersymmetry: violationbackgroundnew physics: search forMajorana Neutrinoneutriinotsensitivityviolation: LorentzMajoronComputer Science Applicationscalorimeter: cryogenicselectron: energy spectrumsymmetry: Lorentzydinfysiikka
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Analysis of linear alkylbenzene samples with a camera-based equipment

2017

Nestemäisiä tuikeaineita hyödyntävät ilmaisimet ovat saaneet jalansijaa neutriinofysiikassa viime vuosikymmeninä. Perinteisiin Cherenkovin ilmaisimiin niiden etu on suurempi hiukkasten vuorovaikutuksesta aiheutuvan valon tuotto. Lisäksi edullisten, suhteellisen ympäristöystävällisten ja optisesti kirkkaiden tuikeaineyhdisteiden (bentseenin alkyylijohdannaiset) saatavuus mahdollistaa yhä suurempien ilmaisimien rakennuksen. Nestemäisten tuikeaineiden ongelmana on kuitenkin niiden taipumus kerätä epäpuhtauksia itseensä ja niiden muutosalttius UV-säteilyn ja korkeiden lämpötilojen vaikutuksesta. Muutokset heikentävät tuikeaineiden valon tuottoa, ja siksi nestemäisten tuikeaineiden puhdistusta j…

Callio Labnestemäiset tuikeaineetC14 experimentlinear alkylbenzenebentseeniliquid scintillation counting
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Rayleigh scattering of linear alkylbenzene in large liquid scintillator detectors.

2015

Rayleigh scattering poses an intrinsic limit for the transparency of organic liquid scintillators. This work focuses on the Rayleigh scattering length of linear alkylbenzene (LAB), which will be used as the solvent of the liquid scintillator in the central detector of the Jiangmen Underground Neutrino Observatory. We investigate the anisotropy of the Rayleigh scattering in LAB, showing that the resulting Rayleigh scattering length will be significantly shorter than reported before. Given the same overall light attenuation, this will result in a more efficient transmission of photons through the scintillator, increasing the amount of light collected by the photosensors and thereby the energy…

Chemical Physics (physics.chem-ph)PhysicsPhysics - Instrumentation and DetectorsPhysics::Instrumentation and Detectorsbusiness.industryAttenuationDetectorFOS: Physical sciencesPhotodetectorScattering lengthInstrumentation and Detectors (physics.ins-det)ScintillatorHigh Energy Physics - ExperimentPhysics::Fluid DynamicsHigh Energy Physics - Experiment (hep-ex)symbols.namesakeOpticsPhysics - Chemical PhysicsScintillation countersymbolsRayleigh scatteringbusinessInstrumentationJiangmen Underground Neutrino ObservatoryThe Review of scientific instruments
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Application of fast solvent extraction processes to studies of exotic nuclides

1998

Fast solvent extraction is a chemical separation method, which can be applied to study exotic nuclides. Since about 1970 the SISAK technique, which is an on-line method based on multi-stage solvent extraction separations, has been successfully used to investigate the nuclear properties of β-decaying nuclides with half-lives down to about one second. During the last decade it has become possible to produce transactinide elements in high enough yields to investigate their chemical properties on a one-atom-at-a-time scale. For this purpose it was necessary to improve and change the detection part of the SISAK system in order to be capable to detect spontaneously fissioning and α-decaying nucli…

ChemistryHealth Toxicology and MutagenesisNuclear engineeringLiquid scintillation countingPublic Health Environmental and Occupational HealthAnalytical chemistryTransactinide elementChemical separation methodPollutionAnalytical ChemistryNuclear Energy and EngineeringRadiology Nuclear Medicine and imagingNuclideSolvent extractionSpectroscopyJournal of Radioanalytical and Nuclear Chemistry
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A low-mass dark matter search using ionization signals in XENON100

2016

We perform a low-mass dark matter search using an exposure of 30\,kg$\times$yr with the XENON100 detector. By dropping the requirement of a scintillation signal and using only the ionization signal to determine the interaction energy, we lowered the energy threshold for detection to 0.7\,keV for nuclear recoils. No dark matter detection can be claimed because a complete background model cannot be constructed without a primary scintillation signal. Instead, we compute an upper limit on the WIMP-nucleon scattering cross section under the assumption that every event passing our selection criteria could be a signal event. Using an energy interval from 0.7\,keV to 9.1\,keV, we derive a limit on …

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Physics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsDark matterFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesSignalHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)WIMPIonization0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsPhysicsScintillation010308 nuclear & particles physicsDetectorInstrumentation and Detectors (physics.ins-det)Physics and Astronomy (miscellaneous) DARK MATTER XENON TPC WIMPHigh Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Scintillation counterEnergy (signal processing)Astrophysics - Cosmology and Nongalactic Astrophysics
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Electron-interacting dark matter: Implications from DAMA/LIBRA-phase2 and prospects for liquid xenon detectors and NaI detectors

2019

We investigate the possibility for the direct detection of low-mass (GeV scale) weakly interacting massive particles (WIMP) dark matter in scintillation experiments. Such WIMPs are typically too light to leave appreciable nuclear recoils but may be detected via their scattering off atomic electrons. In particular, the DAMA Collaboration [R. Bernabei et al., Nucl. Phys. At. Energy 19, 307 (2018)] has recently presented strong evidence of an annual modulation in the scintillation rate observed at energies as low as 1 keV. Despite a strong enhancement in the calculated event rate at low energies, we find that an interpretation in terms of electron-interacting WIMPs cannot be consistent with ex…

DAMA/LIBRACosmology and Nongalactic Astrophysics (astro-ph.CO)detector: performancePhysics::Instrumentation and DetectorsDark matterFOS: Physical scienceschemistry.chemical_elementElectron01 natural sciencesWIMP: dark matterNuclear physicsHigh Energy Physics - Phenomenology (hep-ph)XenonWIMP0103 physical sciences010306 general physicsenhancementscintillation counterenergy: lowPhysicsScintillationxenon: liquid010308 nuclear & particles physicsatom: wave functionDAMAmodulationHigh Energy Physics - Phenomenologychemistryelectron: scatteringWeakly interacting massive particles[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]direct detection[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Event (particle physics)Astrophysics and astroparticle physicsAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review
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